A dataset provided by the European Space Agency

Name 7375
Title Spiral Structure and OB Star Formation in M51
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=7375;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-to41d4i
Author Scoville, Nicholas Z.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=7375&mission=hst
Publication
  • ACS imaging of star clusters in M 51. I. Identification and radius distribution
  • Clues to the Formation of Spiral Structure in M51 from the Ages and Locations of Star Clusters
  • Detection of Dense Molecular Gas in Interarm Spurs in M51
  • Discovery of Five Candidate Analogs for e Carinae in Nearby Galaxies
  • Hierarchical star formation in M 51: star/cluster complexes
  • High-Mass, OB Star Formation in M51: Hubble Space Telescope Ha and Paa Imaging
  • Multi-transition Study of M51S Molecular Gas Spiral Arms
  • New Constraints on Mass-dependent Disruption of Star Clusters in M51
  • Properties of Resolved Star Clusters in M51
  • Star Formation in NGC 5194 (M51a). II. The Spatially Resolved Star Formation Law
  • Star Formation in NGC 5194 (M51a): The Panchromatic View from GALEX to Spitzer
  • The Age, Mass, and Size Distributions of Star Clusters in M51
  • The Fraction of Stars That Form in Clusters in Different Galaxies
  • The Globular Cluster Systems of Five Nearby Spiral Galaxies: New Insights from Hubble Space Telescope Imaging
  • The Link between the Formation Rates of Clusters and Stars in Galaxies
  • The luminosity function of young star clusters: implications for the maximum mass and luminosity of clusters
  • The progenitor of SN 2005cs in the Whirlpool Galaxy
  • The Star Cluster Mass-Galactocentric Radius Relation: Implications for Cluster Formation
  • The star cluster population of M 51. II. Age distribution and relations among the derived parameters
  • The star cluster population of M 51. III. Cluster disruption and formation history
  • The structure and environment of young stellar clusters in spiral galaxies
  • The young star cluster population of M51 with LEGUS - I. A comprehensive study of cluster formation and evolution
  • Tracing star cluster formation in the interacting galaxy M51
  • Vestige of the Star Cluster Burst in M51
Instrument WFPC2, WFPC2/PC
Temporal Coverage 1999-07-21T05:58:13Z/1999-07-21T11:04:33Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2000-07-22T04:06:51Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Scoville et al., 2000, 'Spiral Structure and OB Star Formation in M51', 1.0, European Space Agency, https://doi.org/10.5270/esa-to41d4i